The
COsmic
Background Explorer (COBE) satellite was launched into space
on November 18, 1989. Its purpose is to measure the infrared and
microwave background radiation created in the early universe. (1)
A Far Infrared Absolute Spectrophotometer (FIRAS) to measure background
radiation's spectrum for comparison with a precise blackbody;
(2) a Differential Microwave Radiometer
(DMR) to map small variations in the background radiation; and
(3) a Diffuse Infrared
Background Experiment (DIRBE) to measure the infrared tail of
the background radiation. It also provided a great deal of informtion
about our own galaxy.
The COBE datasets were developed by the NASA Goddard Space Flight Center under the guidance of the COBE Science Working Group and were provided by the NSSDC. |
The star chart background was produced on a Macintosh with the Voyager II program,
and are ©1988-93 Carina Software,
830 Williams St., San Leandro, CA 94577, (510) 352-7328. Used under license.
©1996-1999 Scott
R. Anderson Last update: 1999 December 6 Please send questions, comments, suggestions, or corrections to srca@mindspring.com. The material on this website may be reused as described under the Open Course License. The Gateway to Educational Materials (GEM) is the key to one-stop, any-stop access to thousands of high quality lesson plans, curriculum units and other education resources on the Internet! GEM is a project of the U.S. Department of Education. The Introduction to Astronomy Webbook is catalogued in the Gateway, and Scott R. Anderson is a member of the GEM Consortium. |